three small transiting planets around the M1V star LP 358-499 have been announced (Wells et al. 2017). These are not included in TEPCat because they fail one of the criteria for inclusion: there is no adequate error analysis for any of the measured properties of the system.

2017/09/05:

mass measurements and revised properties for the two planets in the HD 106315 system (Barros et al. 2017)

2017/09/04:

I recently noticed that WASP-86 and KELT-12 are the same object. They were in fact announced on arXiv on successive days (2016/08/16 for WASP-86, 2016/08/17 for KELT-12). An inspection of the discovery papers shows that the RVs are better for WASP-86, the light curves are better for KELT-12, and that the SuperWASP consortium started to obtain dedicated follow-up photometry well before the KELT team (2013/07/16 versus 2014/08/07). Based on this, the system will be called WASP-86 in TEPCat. KELT-12 has therefore been removed from the catalogue.

added extra zeros to the names of some K2, Kepler and WASP planets, e.g. Kepler-05 becomes Kepler-005 and WASP-80 becomes WASP-080. These changes are visible in the ascii and csv datafiles but not the html tables.

KELT-20 is also called MASCARA-2 (Talens et al. 2017) and the two discovery papers were on arXiv on the same day

2017/07/07:

I have used the name KELT-20 for TEPCat because the KELT discovery paper has more extensive data and analysis, and the KELT team identified this object as a planet candidate significantly earlier than the MASCARA team

added a large number of K2 planets from Crossfield et al. (2016) (finally). A false positive probability of <0.003 was required (i.e. planet confirmation to 3σ or more), and entries for planets in this work but already listed in TEPCat were not modified. Therefore a total of 58 planets was included, out of the 104 validated planets presented in the paper.

the physical properties HTML table now contains calculated values of a, logg, ρ*, gp, ρp and Teq if any of these quantities is not available from published papers but can be calculated from other quantities which are